2024-03-08 |
hst_1144.pmap |
operational |
The ACS WFC bias, dark, CTE dark, and sink files were generated following the ACS WFC anneal on February 26, 2024, and should be used to calibrate ACS WFC observations taken between January 30, 2024 and February 26, 2024. |
2024-03-08 |
hst_1143.pmap |
archived |
New synphot TMC and TMG files were delivered to update the ROMAN WFI element name from W146 to F146. New ROMAN WFI throughput reference files were also delivered to match the ones used by Webbpsf and Pandeia. |
2024-02-19 |
hst_1140.pmap |
archived |
A new post-flash reference file, FLSHFILE, is being delivered because new post-flash calibration data was taken in Nov 2023 as part of proposal 17343. The raw darks were separated by EXPTIME and FLASHDUR and combined with ACSREJ to create short and long-flashed superdarks. These superdarks were differenced and scaled to create an intermediate data product that was then smoothed with a local median filter and renormalized to produce the final post-flash reference file. This reference file is to be used in the calibration of post-flashed data taken after July 01 2023. |
2024-02-15 |
hst_1139.pmap |
archived |
The ACS WFC bias, dark, CTE dark, and sink files were generated following the ACS WFC anneal on January 30, 2024, and should be used to calibrate ACS WFC observations taken between January 5, 2024 and January 30, 2024. |